High energy QCD scattering, the shape of gravity on an IR brane, and the Froissart bound

Details High energy QCD scattering, the shape of gravity on an IR brane, and the Froissart bound High energy QCD scattering, the shape of gravity on an IR brane, and the Froissart bound

2002-03-01

arxiv.org/abs/hep-th/0203004v3

Phys.Rev.D67:126001,2003

Physics

High Energy Physics

High Energy Physics - Theory

27 pages, 1 fig, harvmac. v2: references added, typos corrected v3: typo corrected

Scientific paper

10.1103/PhysRevD.67.126001

High-energy scattering in non-conformal gauge theories is investigated using the AdS/CFT dual string/gravity theory. It is argued that strong-gravity processes, such as black hole formation, play an important role in the dual dynamics. Further information about this dynamics is found by performing a linearized analysis of gravity for a mass near an infrared brane; this gives the far field approximation to black hole or other strong-gravity effects, and in particular allows us to estimate their shape. From this shape, one can infer a total scattering cross-section that grows with center of mass energy as ln^2 E, saturating the Froissart bound.

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